Early scrambling and capped BTZ geometries
Abstract
Geodesic probes in certain horizonless microstate geometries experience extreme tidal forces long before reaching the region where these geometries differ significantl from the extremal BTZ black hole. The purpose of this paper is to show that this behavior is a universal feature of all geometries that have a long BTZ throat that terminates in a cap, regardless of the details of this cap. Hence, incoming probes will scramble into the microstate structure before they encounter the region where the charges of the solution are sourced, and the reason for this premature scrambling is the amplification of tiny geometrical deviations by the relativistic speeds of the probes. To illustrate the phenomenon, we construct a new family of smooth horizonless superstratum microstate geometries, dual to D1-D5 CFT states whose momentum charge is carried by excitations on CFT strands of length k. We also show that, in the large-k limit, these new superstrata resemble a blackened supertube solution everywhere except in the near-supertube region. Thus they resolve the singularity caused by the naive back-reaction of modes with non-linear instabilities near evanescent ergosurfaces.
- Authors:
-
- Univ. Paris-Saclay, Gif-sur-Yvette (France)
- Univ. of Chicago, IL (United States)
- Univ. of Southern California, Los Angeles, CA (United States)
- Publication Date:
- Research Org.:
- Univ. of Chicago, IL (United States); Univ. of Southern California, Los Angeles, CA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC); John Templeton Foundation; Agence National de la Recherche (ANR)
- OSTI Identifier:
- 1611254
- Grant/Contract Number:
- SC0009924; SC0011687; ANR-16-CE31-0004-01; 61169
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Journal of High Energy Physics (Online)
- Additional Journal Information:
- Journal Name: Journal of High Energy Physics (Online); Journal Volume: 2019; Journal Issue: 4; Journal ID: ISSN 1029-8479
- Publisher:
- Springer Berlin
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; 79 ASTRONOMY AND ASTROPHYSICS; physics; black holes in string theory; AdS-CFT correspondence
Citation Formats
Bena, Iosif, Martinec, Emil J., Walker, Robert, and Warner, Nicholas P. Early scrambling and capped BTZ geometries. United States: N. p., 2019.
Web. doi:10.1007/jhep04(2019)126.
Bena, Iosif, Martinec, Emil J., Walker, Robert, & Warner, Nicholas P. Early scrambling and capped BTZ geometries. United States. https://doi.org/10.1007/jhep04(2019)126
Bena, Iosif, Martinec, Emil J., Walker, Robert, and Warner, Nicholas P. Fri .
"Early scrambling and capped BTZ geometries". United States. https://doi.org/10.1007/jhep04(2019)126. https://www.osti.gov/servlets/purl/1611254.
@article{osti_1611254,
title = {Early scrambling and capped BTZ geometries},
author = {Bena, Iosif and Martinec, Emil J. and Walker, Robert and Warner, Nicholas P.},
abstractNote = {Geodesic probes in certain horizonless microstate geometries experience extreme tidal forces long before reaching the region where these geometries differ significantl from the extremal BTZ black hole. The purpose of this paper is to show that this behavior is a universal feature of all geometries that have a long BTZ throat that terminates in a cap, regardless of the details of this cap. Hence, incoming probes will scramble into the microstate structure before they encounter the region where the charges of the solution are sourced, and the reason for this premature scrambling is the amplification of tiny geometrical deviations by the relativistic speeds of the probes. To illustrate the phenomenon, we construct a new family of smooth horizonless superstratum microstate geometries, dual to D1-D5 CFT states whose momentum charge is carried by excitations on CFT strands of length k. We also show that, in the large-k limit, these new superstrata resemble a blackened supertube solution everywhere except in the near-supertube region. Thus they resolve the singularity caused by the naive back-reaction of modes with non-linear instabilities near evanescent ergosurfaces.},
doi = {10.1007/jhep04(2019)126},
journal = {Journal of High Energy Physics (Online)},
number = 4,
volume = 2019,
place = {United States},
year = {Fri Apr 19 00:00:00 EDT 2019},
month = {Fri Apr 19 00:00:00 EDT 2019}
}
Web of Science
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Works referencing / citing this record:
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